Cargando…
Linear Isentropic Oscillations of Stars Theoretical Foundations /
The study of stellar oscillations is the preeminent way to investigate the stability of stars and to interpret their variability. The theory of the linear, isentropic oscillations of isolated gaseous stars, and thus of compressible spherically symmetric equilibrium configurations, has largely been d...
| Clasificación: | Libro Electrónico |
|---|---|
| Autores principales: | , |
| Autor Corporativo: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Berlin, Heidelberg :
Springer Berlin Heidelberg : Imprint: Springer,
2010.
|
| Edición: | 1st ed. 2010. |
| Colección: | Astrophysics and Space Science Library,
371 |
| Temas: | |
| Acceso en línea: | Texto Completo |
MARC
| LEADER | 00000nam a22000005i 4500 | ||
|---|---|---|---|
| 001 | 978-3-642-13030-4 | ||
| 003 | DE-He213 | ||
| 005 | 20220113024058.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 110114s2010 gw | s |||| 0|eng d | ||
| 020 | |a 9783642130304 |9 978-3-642-13030-4 | ||
| 024 | 7 | |a 10.1007/978-3-642-13030-4 |2 doi | |
| 050 | 4 | |a QB500.5-785 | |
| 072 | 7 | |a PHV |2 bicssc | |
| 072 | 7 | |a PGS |2 bicssc | |
| 072 | 7 | |a SCI005000 |2 bisacsh | |
| 072 | 7 | |a PHV |2 thema | |
| 072 | 7 | |a PGS |2 thema | |
| 082 | 0 | 4 | |a 523.2 |2 23 |
| 100 | 1 | |a Smeyers, Paul. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 0 | |a Linear Isentropic Oscillations of Stars |h [electronic resource] : |b Theoretical Foundations / |c by Paul Smeyers, Tim Van Hoolst. |
| 250 | |a 1st ed. 2010. | ||
| 264 | 1 | |a Berlin, Heidelberg : |b Springer Berlin Heidelberg : |b Imprint: Springer, |c 2010. | |
| 300 | |a XIV, 473 p. |b online resource. | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file |b PDF |2 rda | ||
| 490 | 1 | |a Astrophysics and Space Science Library, |x 2214-7985 ; |v 371 | |
| 505 | 0 | |a Basic Concepts -- The Equations Governing Linear Perturbations in a Quasi-Static Star -- Deviations from the Hydrostatic and Thermal Equilibrium in a Quasi-Static Star -- Eigenvalue Problem of the Linear, Isentropic Normal Modes in a Quasi-Static Star -- Spheroidal and Toroidal Normal Modes -- Determination of Spheroidal Normal Modes: Mathematical Aspects -- The Eulerian Perturbation of the Gravitational Potential -- The Variational Principle of Hamilton -- Radial Propagation of Waves -- Classification of the Spheroidal Normal Modes -- Classification of the Spheroidal Normal Modes (continued) -- Completeness of the Linear, Isentropic Normal Modes -- N 2(r) Nowhere Negative as Condition for Non-Radial Modes with Real Eigenfrequencies -- Asymptotic Representation of Low-Degree, Higher-Order p-Modes -- Asymptotic Representation of Low-Degree and Intermediate-Degree p-Modes -- Asymptotic Representation of Low-Degree, Higher-Order g +-Modes in Stars Containing a Convective Core -- Asymptotic Representation of Low-Degree, Higher-Order g +-Modes in Stars Consisting of a Radiative Core and a Convective Envelope -- High-Degree, Low-Order Modes -- Period Changes in a Rapidly Evolving Pulsating Star. | |
| 520 | |a The study of stellar oscillations is the preeminent way to investigate the stability of stars and to interpret their variability. The theory of the linear, isentropic oscillations of isolated gaseous stars, and thus of compressible spherically symmetric equilibrium configurations, has largely been developed from the viewpoint of the hypothesis of the physical radial pulsations of stars. Written for doctoral students and researchers, this monograph aims to provide a systematic and consistent survey of the fundamentals of the theory of free, linear, isentropic oscillations in spherically symmetric, gaseous equilibrium stars. The first part of the book presents basic concepts and equations, the distinction between spheroidal and toroidal normal modes, the solution of Poisson's differential equation for the perturbation of the gravitational potential, and Hamilton's variational principle. The second part is devoted to the possible existence of waves propagating in the radial direction, the origin and classification of normal modes, the completeness of the normal modes, and the relation between the local stability with respect to convection and the global stability of a star. The third part deals with asymptotic representations of normal modes and with slow period changes in rapidly evolving pulsating stars. | ||
| 650 | 0 | |a Solar system. | |
| 650 | 0 | |a Astrophysics. | |
| 650 | 0 | |a Mechanics. | |
| 650 | 0 | |a Thermodynamics. | |
| 650 | 0 | |a Acoustics. | |
| 650 | 1 | 4 | |a Space Physics. |
| 650 | 2 | 4 | |a Astrophysics. |
| 650 | 2 | 4 | |a Classical Mechanics. |
| 650 | 2 | 4 | |a Thermodynamics. |
| 650 | 2 | 4 | |a Acoustics. |
| 700 | 1 | |a Van Hoolst, Tim. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 710 | 2 | |a SpringerLink (Online service) | |
| 773 | 0 | |t Springer Nature eBook | |
| 776 | 0 | 8 | |i Printed edition: |z 9783642130298 |
| 776 | 0 | 8 | |i Printed edition: |z 9783642266126 |
| 776 | 0 | 8 | |i Printed edition: |z 9783642130311 |
| 830 | 0 | |a Astrophysics and Space Science Library, |x 2214-7985 ; |v 371 | |
| 856 | 4 | 0 | |u https://doi.uam.elogim.com/10.1007/978-3-642-13030-4 |z Texto Completo |
| 912 | |a ZDB-2-PHA | ||
| 912 | |a ZDB-2-SXP | ||
| 950 | |a Physics and Astronomy (SpringerNature-11651) | ||
| 950 | |a Physics and Astronomy (R0) (SpringerNature-43715) | ||